Non-thermal emission in the core of Perseus: Results from a long XMM-Newton observation

Astronomy and Astrophysics

Volumn 493, Issue 1, 2009, Pages 13-21

  Molendi, S ^a   Gastaldello, F ^b,c,d  

^a INAF IASF MILANO   (Italy)

^b UNIVERSITY OF BOLOGNA   (Italy)

^c OSSERVATORIO ASTRONOMICO DI BOLOGNA   (Italy)

^d UNIVERSITY OF CALIFORNIA   (United States)

Author keywords

Galaxies: clusters: general; Galaxies: clusters: individual: Perseus; X rays: galaxies: clusters

Indexed keywords

MAGNETIC FIELDS; OBSERVATORIES; SURFACE TREATMENT; SYSTEMATIC ERRORS;

CHANDRA; EFFECTIVE AREAS; FARADAY ROTATIONS; GALAXIES: CLUSTERS: GENERAL; GALAXIES: CLUSTERS: INDIVIDUAL: PERSEUS; LOWER LIMITS; METICULOUS ANALYSES; MINIMUM ENERGIES; NEWTON OBSERVATIONS; SURFACE BRIGHTNESSES; THERMAL EMISSIONS; X-RAYS: GALAXIES: CLUSTERS;

GALAXIES;

EID: 58149313933     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:200810138     Document Type: Article

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